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Determination of the amplitude of the repulsive-apir potential between particles clothed by end-grafted polymers

机译:确定末端接枝聚合物覆盖的颗粒之间排斥排斥电位的幅度

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We examine the problem of the determination of the repulsive potential between spherical particles clothed by long end-grafted flexible polymers. This potential varying with the distance according to a logarithmic law has a potential amplitude that depends on the number, L, of grafting chains per particle. The purpose of this work is to compute such a potential amplitude. The clothed particles are first regarded as star polymers with small enough diameter and the same number of arms. Then, the amplitude potential is identified to the critical exponent related to the contact probability between cores of these stars, which allows us to find a universal function for the expected potential amplitude depending on L and d-space dimension only. In two-dimensional space, conformal invariance is used to extract the potential amplitude as a function of L. For dimensions greater than 2, the potential amplitude is obtained within the framework of renormalization theory to third order in #epsilon# = 4-d, where d is the critical dimension of the system. To determine the best three-dimensional expression for the potential amplitude, A_L, use is made of the Pade-Borel transformation, which provides a closer form valid for small, intermediate and high values of L. This form of potential amplitude, consistent with the exact scaling asymptotic value of Witten and Pincus [(1986) Macromolecules 19:2509], allows us to find the associated prefactor. The procedure is also extended to interacting stars of different number of arms.
机译:我们研究了确定由长端接枝的柔性聚合物覆盖的球形颗粒之间的排斥势的问题。根据对数定律,该电势随距离而变化,其电势幅度取决于每个粒子的接枝链数L。这项工作的目的是计算这样的电位幅度。首先将被覆盖的颗粒视为具有足够小的直径和相同数量的臂的星形聚合物。然后,将振幅电势识别为与这些恒星的核之间的接触概率有关的临界指数,这使我们能够仅根据L空间和d空间维来找到预期电势振幅的通用函数。在二维空间中,使用共形不变性提取作为L的函数的势振幅。对于大于2的维,在#epsilon#= 4-d的重归一化理论框架内获得三阶势振幅。 d是系统的关键尺寸。为了确定势振幅A_L的最佳三维表达式,使用了Pade-Borel变换,该变换提供了一种更接近的形式,适用于L的小,中和高值。这种形式的势振幅与Witten和Pincus的精确缩放渐近值[(1986)Macromolecules 19:2509],使我们能够找到相关的前置因子。该程序还扩展到了具有不同臂数的相互作用恒星。

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